SPIRAL ROTATION IN RAYLEIGH-BENARD
CONVECTION
(simulation of the Swift-Hohenberg
equation coupled with mean flow)
Spiral terminated by a dislocation
Snapshots every 10 units of time:
Here is a movie
(50 kB) of spiral rotation. Watch how the spiral quickly winds up first,
and then the frequency of core rotation becomes smaller than dislocation's.
lev@gibbs.ucsd.edu